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Search for low-mass dark matter WIMPs with 12 ton-day exposure of DarkSide-50

Authors :
Agnes, P.
Albuquerque, I.F.M.
Alexander, T.
Alton, A.K.
Ave, M.
Back, H.O.
Batignani, G.
Biery, K.
Bocci, V.
Bonivento, W.M.
Bottino, B.
Bussino, S.
Cadeddu, M.
Cadoni, M.
Calaprice, F.
Caminata, A.
Campos, M.D.
Canci, N.
Caravati, M.
Cariello, M.
Carlini, M.
Carpinelli, M.
Cataudella, V.
Cavalcante, P.
Cavuoti, S.
Chashin, S.
Chepurnov, A.
Cicalò, C.
Covone, G.
d'Angelo, D.
Davini, S.
de Candia, A.
de Cecco, S.
de Filippis, G.
de Rosa, G.
Derbin, A.V.
Devoto, A.
d'Incecco, M.
Dionisi, C.
Dordei, F.
Downing, M.
d'Urso, D.
Fairbairn, M.
Fiorillo, G.
Franco, D.
Gabriele, F.
Galbiati, C.
Ghiano, C.
Giganti, C.
Giovanetti, G.K.
Goretti, A.M.
Di Cortona, G. Grilli
Grobov, A.
Gromov, M.
Guan, M.
Gulino, M.
Hackett, B.R.
Herner, K.
Hessel, T.
Hosseini, B.
Hubaut, F.
Hungerford, E.V.
Ianni, An.
Ippolito, V.
Keeter, K.
Kendziora, C.L.
Kimura, M.
Kochanek, I.
Korablev, D.
Korga, G.
Kubankin, A.
Kuss, M.
La Commara, M.
Lai, M.
Li, X.
Lissia, M.
Longo, G.
Lychagina, O.
Machulin, I.N.
Mapelli, L.P.
Mari, S.M.
Maricic, J.
Martoff, C.J.
Messina, A.
Milincic, R.
Monroe, J.
Morrocchi, M.
Mougeot, X.
Muratova, V.N.
Musico, P.
Nozdrina, A.O.
Oleinik, A.
Ortica, F.
Pagani, L.
Pallavicini, M.
Pandola, L.
Pantic, E.
Paoloni, E.
Pelczar, K.
Pelliccia, N.
Piacentini, S.
Picciau, E.
Pocar, A.
Poehlmann, D.M.
Pordes, S.
Poudel, S.S.
Pralavorio, P.
Price, D.D.
Ragusa, F.
Razeti, M.
Razeto, A.
Renshaw, A.L.
Rescigno, M.
Rode, J.
Romani, A.
Sablone, D.
Samoylov, O.
Sands, W.
Sanfilippo, S.
Sanford, E.
Savarese, C.
Schlitzer, B.
Semenov, D.A.
Shchagin, A.
Sheshukov, A.
Skorokhvatov, M.D.
Smirnov, O.
Sotnikov, A.
Stracka, S.
Suvorov, Y.
Tartaglia, R.
Testera, G.
Tonazzo, A.
Unzhakov, E.V.
Vishneva, A.
Vogelaar, R.B.
Wada, M.
Wang, H.
Wang, Y.
Westerdale, S.
Wojcik, M.M.
Xiao, X.
Yang, C.
Zuzel, G.
Agnes, P.
Albuquerque, I. F. M.
Alexander, T.
Alton, A. K.
Ave, M.
Back, H. O.
Batignani, G.
Biery, K.
Bocci, V.
Bonivento, W. M.
Bottino, B.
Bussino, S.
Cadeddu, M.
Cadoni, M.
Calaprice, F.
Caminata, A.
Canci, N.
Caravati, M.
Cargioli, N.
Cariello, M.
Carlini, M.
Cataudella, V.
Cavalcante, P.
Cavuoti, S.
Chashin, S.
Chepurnov, A.
Cicalò, C.
Covone, G.
D’Angelo, D.
Davini, S.
De Candia, A.
De Cecco, S.
De Filippis, G.
De Rosa, G.
Derbin, A. V.
Devoto, A.
D’Incecco, M.
Dionisi, C.
Dordei, F.
Downing, M.
D’Urso, D.
Fiorillo, G.
Franco, D.
Gabriele, F.
Galbiati, C.
Ghiano, C.
Giganti, C.
Giovanetti, G. K.
Goretti, A. M.
Grilli di Cortona, G.
Grobov, A.
Gromov, M.
Guan, M.
Gulino, M.
Hackett, B. R.
Herner, K.
Hessel, T.
Hosseini, B.
Hubaut, F.
Hungerford, E. V.
Ianni, An.
Ippolito, V.
Keeter, K.
Kendziora, C. L.
Kimura, M.
Kochanek, I.
Korablev, D.
Korga, G.
Kubankin, A.
Kuss, M.
La Commara, M.
Lai, M.
Li, X.
Lissia, M.
Longo, G.
Lychagina, O.
Machulin, I. N.
Mapelli, L. P.
Mari, S. M.
Maricic, J.
Messina, A.
Milincic, R.
Monroe, J.
Morrocchi, M.
Mougeot, X.
Muratova, V. N.
Musico, P.
Nozdrina, A. O.
Oleinik, A.
Ortica, F.
Pagani, L.
Pallavicini, M.
Pandola, L.
Pantic, E.
Paoloni, E.
Pelczar, K.
Pelliccia, N.
Piacentini, S.
Pocar, A.
Poehlmann, D. M.
Pordes, S.
Poudel, S. S.
Pralavorio, P.
Price, D. D.
Ragusa, F.
Razeti, M.
Razeto, A.
Renshaw, A. L.
Rescigno, M.
Rode, J.
Romani, A.
Sablone, D.
Samoylov, O.
Sands, W.
Sanfilippo, S.
Sandford, E.
Savarese, C.
Schlitzer, B.
Semenov, D. A.
Shchagin, A.
Sheshukov, A.
Skorokhvatov, M. D.
Smirnov, O.
Sotnikov, A.
Stracka, S.
Suvorov, Y.
Tartaglia, R.
Testera, G.
Tonazzo, A.
Unzhakov, E. V.
Vishneva, A.
Vogelaar, R. B.
Wada, M.
Wang, H.
Wang, Y.
Westerdale, S.
Wojcik, M. M.
Xiao, X.
Yang, C.
Zuzel, G.
Royal Holloway [University of London] (RHUL)
Universidade de São Paulo = University of São Paulo (USP)
Pacific Northwest National Laboratory (PNNL)
University of South Dakota [Vermillion] (USD)
Istituto Nazionale di Fisica Nucleare [Pisa] (INFN)
Istituto Nazionale di Fisica Nucleare (INFN)
Fermi National Accelerator Laboratory (Fermilab)
Istituto Nazionale di Fisica Nucleare [Sezione di Roma 1] (INFN)
Istituto Nazionale di Fisica Nucleare
Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari (INFN, Sezione di Cagliari)
Università degli studi di Genova = University of Genoa (UniGe)
Princeton University
Istituto Nazionale di Fisica Nucleare, Sezione di Genova (INFN, Sezione di Genova)
Gran Sasso Science Institute, INFN
University of Naples Federico II = Università degli studi di Napoli Federico II
Virginia Tech [Blacksburg]
D.V. Skobeltsyn Institute of Nuclear Physics (SINP)
Lomonosov Moscow State University (MSU)
Istituto Nazionale di Fisica Nucleare, Sezione di Milano (INFN)
Università degli Studi di Cagliari = University of Cagliari (UniCa)
University of Massachusetts System (UMASS)
Università degli Studi di Sassari = University of Sassari [Sassari] (UNISS)
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (INFN, Sezione di Napoli)
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
INFN Frascati
Institute of Molecular Genetics of National Research Centre «Kurchatov Institute» [Moscow, Russia]
Russian Academy of Sciences [Moscow] (RAS)
Institute of High Energy Physics [Beijing] (IHEP)
Chinese Academy of Sciences [Changchun Branch] (CAS)
Università degli Studi di Enna ' KORE ' = Kore University of Enna
Centre de Physique des Particules de Marseille (CPPM)
Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
University of Houston
Black Hills State University
Nicolaus Copernicus Astronomical Cente (AstroCeNT)
Joint Institute for Nuclear Research (JINR)
Belgorod National Research University
University of California [Los Angeles] (UCLA)
University of California (UC)
University of Hawai'i [Hilo]
Laboratoire National Henri Becquerel (LNHB)
Département Métrologie Instrumentation & Information (DM2I)
Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA))
Direction de Recherche Technologique (CEA) (DRT (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département d'instrumentation Numérique (DIN (CEA-LIST))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Università degli Studi di Perugia = University of Perugia (UNIPG)
Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN)
Università degli studi di Catania = University of Catania (Unict)
INFN Laboratori Nazionali del Gran Sasso
University of Massachusetts [Amherst] (UMass Amherst)
University of Manchester [Manchester]
Università degli Studi di Milano = University of Milan (UNIMI)
Università degli Studi Roma Tre = Roma Tre University (ROMA TRE)
Moscow State Engineering Physics Institute (MEPhI)
Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA)
Nicolaus Copernicus Astronomical Center (AstroCENT)
Uniwersytet Jagielloński w Krakowie = Jagiellonian University (UJ)
SCOAP
DarkSide-50
HEP, INSPIRE
Source :
Physical Review, Physical Review D, Physical Review D, 2023, 107 (6), pp.063001. ⟨10.1103/PhysRevD.107.063001⟩, Phys.Rev.D, Phys.Rev.D, 2023, 107 (6), pp.063001
Publication Year :
2023

Abstract

We report on the search for dark matter WIMPs in the mass range below 10 GeV/c$^2$, from the analysis of the entire dataset acquired with a low-radioactivity argon target by the DarkSide-50 experiment at LNGS. The new analysis benefits from more accurate calibration of the detector response, improved background model, and better determination of systematic uncertainties, allowing us to accurately model the background rate and spectra down to 0.06 keV$_{er}$. A 90% C.L. exclusion limit for the spin-independent cross section of 3 GeV/c$^2$ mass WIMP on nucleons is set at 6$\times$10$^{-43}$ cm$^2$, about a factor 10 better than the previous DarkSide-50 limit. This analysis extends the exclusion region for spin-independent dark matter interactions below the current experimental constraints in the $[1.2, 3.6]$ GeV/c$^2$ WIMP mass range.<br />11 pages, 12 figures

Details

Language :
English
ISSN :
15507998 and 15502368
Database :
OpenAIRE
Journal :
Physical Review, Physical Review D, Physical Review D, 2023, 107 (6), pp.063001. ⟨10.1103/PhysRevD.107.063001⟩, Phys.Rev.D, Phys.Rev.D, 2023, 107 (6), pp.063001
Accession number :
edsair.doi.dedup.....ddbcb0b71f43e934cb68b63e9bdf8780